Yanagisawa, Hiroto https://orcid.org/0009-0006-6763-4245
Ouchi, Masami https://orcid.org/0000-0002-1049-6658
Nakajima, Kimihiko https://orcid.org/0000-0003-2965-5070
Harikane, Yuichi https://orcid.org/0000-0002-6047-430X
Fujimoto, Seiji https://orcid.org/0000-0001-7201-5066
Ono, Yoshiaki https://orcid.org/0000-0001-9011-7605
Umeda, Hiroya https://orcid.org/0009-0008-0167-5129
Nakane, Minami https://orcid.org/0009-0000-1999-5472
Yajima, Hidenobu https://orcid.org/0000-0002-1319-3433
Fukushima, Hajime https://orcid.org/0000-0002-0547-3208
Funding for this research was provided by:
MEXT ∣ Japan Society for the Promotion of Science (20H00180)
MEXT ∣ Japan Society for the Promotion of Science (21H04467)
MEXT ∣ Japan Society for the Promotion of Science (21H04489)
MEXT ∣ Japan Society for the Promotion of Science (24K07102)
MEXT ∣ JST ∣ Fusion Oriented REsearch for disruptive Science and Technology (JP-MJFR202Z)
Article Title: A Galaxy with an Extremely Blue Ultraviolet Slope β = −3 at z = 9.25 Identified by JWST Spectroscopy: Evidence for a Weak Nebular Continuum and Efficient Ionizing Photon Escape?
Journal Title: The Astrophysical Journal
Article Type: paper
Copyright Information: © 2025. The Author(s). Published by the American Astronomical Society.
Publication dates
Date Received: 2024-11-29
Date Accepted: 2025-04-16
Online publication date: 2025-07-15